The Recurrent Eclipsing Nova U Sco: A Short Review

Authors

  • R. González-Riestra XMM Science Operations Centre, ESAC, Madrid, Spain

DOI:

https://doi.org/10.14311/APP.2015.02.0252

Abstract

U Scorpii is the recurrent nova with the shortest inter-outburst period, only ten years. The last active phase took place at the beginning of 2010, and it provided a large amount of data from both ground-based and space observatories. This paper reviews some of the more relevant recent findings and points out some, still unanswered, questions.

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Published

2015-02-23

How to Cite

González-Riestra, R. (2015). The Recurrent Eclipsing Nova U Sco: A Short Review. Acta Polytechnica CTU Proceedings, 2(1), 252–256. https://doi.org/10.14311/APP.2015.02.0252